Photometric Studies of Twelve Deep, Low-mass Ratio Overcontact Binary Systems

The formations of the blue straggler stars and the FK Com-type stars are unsolved problems in stellar astrophysics. One of the possibilities for their formations is from the coalescence of W UMa-type overcontact binary systems. Therefore, deep (f > 50%), low-mass ratio (q < 0.25) overcontact binary stars are a very important source to understand the phenomena of Blue Straggler/FK Com-type stars. Recently, 12 W UMa-type binary stars, FG Hya, GR Vir, IK Per, TV Mus, CU Tau, V857 Her, V410 Aur, XY Boo, SX CrV, QX And, GSC 619-232, and AH Cnc, were investigated photometrically. Apart from TV Mus, XY boo, and GSC 619-232, new observations of the other 9 binaries were obtained. Complete light curves of the 10 systems, FG Hya, GR Vir, IK Per, TV Mus, CU Tau, V857 Her, GSC 619-232, V410 Aur, XY Boo, and AH Cnc, were analyzed with the 2003 version of the W-D code. It is shown that all of those systems are deep (f > 50%), low-mass ratio (q < 0.25) overcontact binary stars. We found that the system GSC 619-232 has the highest degree of overcontact (f = 93.4%). The derived photometric mass ratio of V857 Her, q = 0.0653, indicates that it is the lowest-mass ratio system among W UMa-type binaries.Of the 12 sample stars, long-term period changes of 11 systems were found. About 58% (seven) of the sample binaries show cyclic period oscillation. No cyclic period changes were discovered for the other 5 systems, which may be caused by the short observational time interval or by insufficient observations. Therefore, we think that all W UMa-type binary stars may contain cyclic period variations. By considering the long-term period changes (both increase and decrease) of those binary stars, we proposed two evolutionary scenarios evolving from deep, low-mass ratio overcontact binaries into Blue Straggler/FK Com-type stars.     

不同地壳速度结构对安徽地区地震定位深度的影响

地震深度定位对地壳速度结构模型有较大的依赖性。选取2017年安徽及周边M_L 1.5以上地震,使用PTD与单纯型定位方法,分别配置华南模型与AH2015模型进行重新定位,研究不同模型对安徽地震深度的定位影响。研究表明,使用PTD方法,配置AH2015模型时定位深度略大,且符合安徽区域地震实际深度的记录台站较多;使用单纯型定位法,配置两种模型所得定位深度差距不大,且深度分布均匀。说明PTD方法定位地震深度对地壳速度结构模型的依赖程度较大,AH2015模型比华南模型更加符合安徽区域实际地壳结构。     

广州人为热初步估算及敏感性分析

考虑了工业、交通和生活三种人为热排放源,利用广州市工业和生活能源消耗量、汽车保有量、主干道车流量等数据,估算出广州人为热日变化排放通量,全天平均排放通量411 W〖DK〗·m-2,最大排放通量出现在11时,为723 W ·m-2,其中工业排放占总排放量686%。利用耦合到WRF中的单层城市冠层模式(WRF/UCM),对人为热作用进行敏感性试验,包括无人为热、无日变化人为热、有日变化人为热、人为热排放通量翻倍四种方案。结果显示,方案之间冠层感热通量的差异与人为热设置的差异大致相等。试验方案之间冠层内气温差异较小,单倍人为热与双倍人为热的最大差值约只有02℃。另外,人为热使湍流得到发展,双倍人为热比单倍人为热湍流动能增加约01~04 m2 ·s-2。且人为热对白天城市边界层湍涡有增强作用,添加单倍人为热后使气流垂直速度最大增加可达01 m ·s-1,使垂直混合加强。有日变化的人为热对热岛强度的贡献在中午时最大,单倍人为热的平均贡献率159%,双倍人为热为228%;而无日变化的人为热在凌晨时贡献最大,平均贡献率149%。     

AH5井区八道湾组砂质和砾质储层孔隙结构特征及评价

准噶尔盆地AH区块侏罗系八道湾组属于低饱和度、特低孔特低渗储层,孔隙结构研究较为模糊,导致储集层产能评价认识不清。为对研究区目的层孔隙结构进行定量化描述及识别,利用岩心观察、普通、荧光、铸体薄片、扫描电镜、高压压汞、岩心油水饱和度、相渗及物性分析等资料对孔隙结构复杂特征进行定量表征及分类,并对相渗特征进行分析。结果表明:八道湾组储层可分为砂质和砾质储层,储层孔隙类型包括剩余粒间孔、粒间和粒内溶孔、铸模孔、微裂缝以及晶间孔,喉道类型包括孔隙缩小型、缩颈型、片状、片弯状以及管束状喉道。在油水饱和度实验分析和压汞基础参数分析基础上,将砂岩和砾岩储层根据分形维数对孔隙结构综合定量划分为Ⅰ—Ⅲ类,砾质储层产能相对砂质储层更好。     

不同地壳速度结构对安徽地区地震定位深度的影响

地震深度定位对地壳速度结构模型有较大的依赖性。选取2017年安徽及周边M_L 1.5以上地震,使用PTD与单纯型定位方法,分别配置华南模型与AH2015模型进行重新定位,研究不同模型对安徽地震深度的定位影响。研究表明,使用PTD方法,配置AH2015模型时定位深度略大,且符合安徽区域地震实际深度的记录台站较多;使用单纯型定位法,配置两种模型所得定位深度差距不大,且深度分布均匀。说明PTD方法定位地震深度对地壳速度结构模型的依赖程度较大,AH2015模型比华南模型更加符合安徽区域实际地壳结构。